Results 121 to 130 of about 280,504 (183)

Association Reaction of Gaseous C₂H₄ in Femtosecond Laser Filaments Studied by Time-of-Flight Mass Spectrometry. [PDF]

ACS Omega, 2021
Matsuda A, Tani K, Takeuchi Y, Hayakawa Y, Hishikawa A.   +4 more
europepmc   +1 more source

Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalog

The Astrophysical Journal Supplement Series
Filaments play a crucial role in providing the necessary environmental conditions for star formation, actively participating in the process. To facilitate the identification and analysis of filaments, we introduce Directional and Positional Consistency ...
Yu Jiang, Xuepeng Chen, Sheng Zheng, Zhibo Jiang, Zhiwei Chen, Yao Huang, Yang Su, Li Sun, Jian-Cheng Feng, Haoran Feng, Ji Yang   +10 more
doaj   +1 more source

Filamentary Hierarchies and Superbubbles. II. Impact of Superbubbles and Galactic Dynamics on Filament Formation and Fragmentation

The Astrophysical Journal
Large-scale phenomena in spiral galaxies such as shear, supernovae, and magnetic fields all contribute to the formation and subsequent evolution of filamentary structure and star formation within them.
Rachel Pillsworth, Ralph E. Pudritz, Eric W. Koch, Theo J. O’Neill   +3 more
doaj   +1 more source

Why Are (Almost) All the Protostellar Outflows Aligned in Serpens Main?

The Astrophysical Journal
We present deep 1.4–4.8 μ m JWST-NIRCam imaging of the Serpens Main star-forming region and identify 20 candidate protostellar outflows, most with bipolar structure and identified driving sources. The outflow position angles (PAs) are strongly correlated,
Joel D. Green, Klaus M. Pontoppidan, Megan Reiter, Dan M. Watson, Sachindev S. Shenoy, P. Manoj, Mayank Narang   +6 more
doaj   +1 more source

Polarized radio filaments outside the Galactic plane

, 2014
We used data from the WMAP satellite at 23, 33 and 41 GHz to study the diffuse polarized emission over the entire sky. The emission originates mostly from filamentary structures with well-ordered magnetic fields.
Leahy, J P, J. P. Leahy, C. Dickinson, Dickinson, C; id_orcid, Vidal, Matias, Davies, R D, M. Vidal, R. D. Davies   +7 more
core  

Tailoring Vibrational Signature and Functionality of 2D-Ordered Linear-Chain Carbon-Based Nanocarriers for Predictive Performance Enhancement of High-End Energetic Materials. [PDF]

Nanomaterials (Basel), 2022
Lukin A, Gülseren O.
europepmc   +1 more source

Polarized radio filaments outside the Galactic plane

, 2015
We used data from the WMAP satellite at 23, 33 and 41 GHz to study the diffuse polarized emission over the entire sky. The emission originates mostly from filamentary structures with well-ordered magnetic fields.
Leahy, J P, Dickinson, C; id_orcid, Vidal, Matias, Davies, R D   +3 more
core  

Probing properties of star forming filaments : an initial investigation of filaments' characteristics using STARFORGE simulation data

Cold dense interstellar gas provides an optimal environment for the formation of stars. These overdense regions or “cores” are generally part of longer thread-like structures known as filaments. Velocity gradients, along and resulting from other physical
Pinedo, Savannah Alexis
core   +1 more source

Considering light-matter interactions in the Friedmann equations. [PDF]

Proc Math Phys Eng Sci, 2022
Vavryčuk V.
europepmc   +1 more source

Complex plasma research under microgravity conditions. [PDF]

NPJ Microgravity, 2023
Thoma MH, Thomas HM, Knapek CA, Melzer A, Konopka U.   +4 more
europepmc   +1 more source